SDO HMI 2011-11-12 14:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.39 | 324.26 | 24.30 | 177.60 | 27.97 | 43.62 | -4.82 | 10.02 | 0.4281 | -933.3 | -402.3 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.55 | 0.00 | 0.85 | 28.47 | 48.85 | 0.41 | 359.15 | 0.4292 | -790.0 | -583.7 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 32.07 | 45.22 | -3.22 | 5.62 | 0.4877 | -748.0 | -655.1 | |
| 40.09 | 312.13 | 21.93 | 170.91 | 27.91 | 43.81 | -4.63 | 9.67 | 0.4264 | -1332.5 | -420.0 | |
| 0.77 | -3.00 | 0.43 | -3.00 | 28.56 | 43.58 | -4.86 | 9.85 | 0.4372 | -761.9 | 999999 | |
| 2.84 | -3.00 | 1.56 | -3.00 | 28.36 | 43.42 | -5.02 | 10.25 | 0.4346 | -878.7 | 999999 | |
| 0.69 | -3.00 | 0.38 | -3.00 | 28.10 | 43.23 | -5.21 | 10.76 | 0.4311 | -876.0 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 29.27 | 41.15 | -7.29 | 14.11 | 0.4560 | -707.0 | -596.3 | |
| 0.00 | 1.98 | 0.00 | 1.10 | 28.61 | 40.62 | -7.82 | 15.53 | 0.4482 | -752.0 | -643.0 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 24.93 | 38.12 | -10.32 | 23.62 | 0.4072 | 707.0 | 582.5 | |
| 0.00 | 1.46 | 0.00 | 0.81 | 28.26 | 37.71 | -10.73 | 21.11 | 0.4573 | 429.0 | 420.6 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 25.24 | 37.73 | -10.71 | 24.06 | 0.4142 | 755.0 | 598.5 | |
| 0.00 | 2.93 | 0.00 | 1.61 | 27.05 | 37.46 | -10.98 | 22.70 | 0.4416 | 415.0 | 403.2 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 27.37 | 37.12 | -11.32 | 23.00 | 0.4482 | 636.0 | 440.7 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |